Fig. 6
Representative [C II] spectra from the three observed regions, the pillar, globule (center position with bulk emission) and IRAS 20306+4005. The double-peaked spectrum from the IRAS source is due to two seperate components at around 4 and 6 km s-1. The [C II] spectrum of the globule (red) shows a shift of around 2 km s-1 with respect to the pillar (blue) and IRAS source (black).
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